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Cited by 463

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

What galaxy surveys really measure

Open access
Bonvin, Camille, Durrer, Ruth·2011·Physical Review D

Abstract

In this paper we compute the quantity which is truly measured in a large galaxy survey. We take into account the effects coming from the fact that we actually observe galaxy redshifts and sky positions and not true spatial positions. Our calculations are done within linear perturbation theory for both the metric and the source velocities but they can be used for nonlinear matter power spectra. We shall see that the complications due to the fact that we only observe on our background light cone, and that we do not truly know the distance of the observed galaxy but only its redshift, not only cause an additional difficulty, but provide even more a new opportunity for future galaxy surveys.

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Metadata

Authors
Bonvin, C., & Durrer, R.
Venue
Physical Review D
Published
2011-09-02
Volume
84
Issue
6
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2024184560
Cited by
463
References
3
FWCI
12.79
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: What galaxy surveys really measure. https://app.cochat.ai/papers/10.1103/physrevd.84.063505
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Bonvin, C., & Durrer, R. (2011). What galaxy surveys really measure. Physical Review D. https://doi.org/10.1103/physrevd.84.063505

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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